Showing 1–20 of 78 results
/ Date/ Name
May 7, 2010Probing New Physics Models of Neutrinoless Double Beta Decay with SuperNEMOSep 29, 2022Search for Cosmic-ray Boosted Sub-GeV Dark Matter using Recoil Protons at Super-KamiokandeJun 3, 2022Search for supernova bursts in Super-Kamiokande IVMar 11, 2024Performance of SK-Gd's Upgraded Real-time Supernova Monitoring SystemOct 30, 2020Search for proton decay via $p\to e^+π^0$ and $p\to μ^+π^0$ with an enlarged fiducial volume in Super-Kamiokande I-IVJan 16, 2019Measurement of neutrino-oxygen neutral-current quasi-elastic cross section using atmospheric neutrinos at Super-KamiokandeJan 10, 2019Atmospheric Neutrino Oscillation Analysis With Improved Event Reconstruction in Super-Kamiokande IVSep 23, 2021Diffuse Supernova Neutrino Background Search at Super-KamiokandeApr 19, 2021Search for neutrinos in coincidence with gravitational wave events from the LIGO-Virgo O3a Observing Run with the Super-Kamiokande detectorFeb 23, 2017The BiPo-3 detector for the measurement of ultra low natural radioactivities of thin materialsDec 20, 2023Solar neutrino measurements using the full data period of Super-Kamiokande-IVSep 18, 2022Neutron Tagging following Atmospheric Neutrino Events in a Water Cherenkov DetectorMay 21, 2024First joint oscillation analysis of Super-Kamiokande atmospheric and T2K accelerator neutrino dataJan 13, 2021Supernova Model Discrimination with Hyper-KamiokandeOct 30, 2025Reconstruction of neutrino events in the Accelerator Neutrino Neutron Interaction Experiment: Part IApr 13, 2026Search for proton decay via $p \to e^{+}π^{0}π^{0}$ and $p \to μ^{+}π^{0}π^{0}$ in 0.401 megaton-years exposure of Super-Kamiokande I-VMay 19, 2022Pre-Supernova Alert System for Super-KamiokandeAug 28, 2022Search for proton decay via $p\rightarrow μ^+K^0$ in 0.37 megaton-years exposure of Super-KamiokandeNov 7, 2023Measurement of the neutrino-oxygen neutral-current quasielastic cross section using atmospheric neutrinos in the SK-Gd experimentOct 24, 2022Searching for neutrinos from solar flares across solar cycles 23 and 24 with the Super-Kamiokande detector